Gravitational waves (GWs) can offer a novel window into the structure and dynamics of
neutron stars. Here we present the first search for long-duration quasimonochromatic GW …

Neutron stars are known to show accelerated spin-up of their rotational frequency called a
glitch. Highly magnetized rotating neutron stars (pulsars) are frequently observed by radio …

Pulsars are spinning neutron stars which emit an electromagnetic beam. We expect pulsars
to slowly decrease their rotational frequency. However, sudden increases of the rotational …

This work explores whether gravitational waves (GWs) from neutron star (NS) mountains can
be detected with current second-generation and future third-generation GW detectors. In …

Pulsars are rotating neutron stars that emit periodic electromagnetic radiation. While pulsars
generally slow down as they lose energy, some also experience glitches: spontaneous …

During their most recent observing run, LIGO/Virgo reported the gravitational wave (GW)
transient S191110af, a burst signal at a frequency of 1.78 kHz that lasted for 0.104 s. While …

Continuous gravitational waves from neutron stars could provide an invaluable resource to
learn about their interior physics. A common search method involves matched filtering a …

Glitching pulsars are expected to be important sources of gravitational waves (GWs). In this
paper, we explore six different models that propose the emission of transient continuous …

Machine learning can be a powerful tool to discover new signal types in astronomical data.
We here apply it to search for long-duration transient gravitational waves triggered by pulsar …

Continuous gravitational waves (CWs) are quasi-monochromatic signals expected to be
ever-present in the data of gravitational-wave (GW) detectors such as Advanced LIGO (Aasi …